Modelling phosphine spectra for the atmospheric characterization of cool stars and exoplanets
Understanding the molecular composition of astrophysical atmospheres depends on the interpretation of their spectra, which is possible through a combination of observational data analysis and computational modelling. However, this process is difficult to perform as the observed spectra have an extre...
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University College London (University of London)
2015
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| Online Access: | https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.745999 |